Nonradial oscillations of Saturn

Details Nonradial oscillations of Saturn Nonradial oscillations of Saturn

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icar...94..420m&link_type=abstract

Icarus (ISSN 0019-1035), vol. 94, Dec. 1991, p. 420-435.

Computer Science

10

Planetary Cores, Saturn Rings, Vibration Mode, Phase Transformations, Planetary Gravitation, Planetary Surfaces

Scientific paper

The planetary interior-state sensitivity of the f-mode oscillations of Saturn, which may be detected through their gravitational signature in the rings, are presently studied in light of the results of mode-period calculations for various interior models, envelope compositions, and hydrogen phase-transition pressures. It is established that the low-degree f modes exhibit the highest sensitivity to the size of the planetary core, while higher-degree modes exhibit greater sensitivity to the rotation state of the Saturn's outer layers.

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